The structure specificity of alpha-chymotrypsin. I. Polypeptides as substrates. II. N-acylated peptide esters as substrates. III. Some reactive esters of N-acylated amino acids as substrates

<p>The structural specificity of α-chymotrypsin for polypeptides and denatured proteins has been examined. The primary specificity of the enzyme for these natural substrates is shown to closely correspond to that observed for model substrates. A pattern of secondary specificity is proposed. p> <p>A series of N-acetylated peptide esters of varying length have been evaluated as substrates of α-chymotrypsin. The results are interpreted in terms of proposed specificity theories. p> <p>The α-chymotrypsin-catalyzed hydrolyses of a number of N-acetylated dipeptide methyl esters were studied. The results are interpreted in terms of the available specificity theories and are compared with results obtained in the study of polypeptide substrates. The importance of non-productive binding in determining the kinetic parameters of these substrates is discussed. A partial model of the locus of the active site which interacts with the R’₁CONH- group of a substrate of the form R’₁CONHCHR₂COR’₃ is proposed.p> <p>Finally, some reactive esters of N-acetylated amino acids have been evaluated as substrates of α-chymotrypsin. Their reactivity and stereo-chemical behavior are discussed in terms of the specificity theories available. The importance of a binding interaction between the carboxyl function of the substrate and the enzyme is suggested by the results obtained. p>

The reduced-alpha-width of the lowest 1¯ state of ^(16)O

<p>Cross sections for the reaction p>12p>C(α,γ)p>16p>O have been measured for a range of center-of-mass alpha particle energies extending from 1.72 MeV to 2.94 MeV. Two 8"x5" NaI (Tℓ) crystals were used to detect gamma rays; time-of-flight technique was employed to suppress cosmic ray background and background due to neutrons arising mainly from the p>13p>C(α,n)p>16p>O reaction. Angular distributions were measured at center-of-mass alpha energies of 2.18, 2.42, 2.56 and 2.83 MeV. Upper limits were placed on the amount of radiation cascading through the 6.92 or 7.12-MeV states in p>16p>O. By means of theoretical fits to the measured electric dipole component of the total cross section, in which interference between the 1¯ states in p>16p>O at 7.12 MeV and at 9.60 MeV is taken into account, it is possible to extract the dimensionless, reduced-alpha-width of the 7.12-MeV state in p>16p>O. A three-level R-matrix parameterization of the data yields the width Θ_α,Fp>2p> = 0.14p>+0.10p>_-0.08. A "hybrid" R-matrix-optical-model parameterization yields Θ_α,Fp>2p> = 0.11p>+0.11p>_-0.07. This quantity is of crucial importance in determining the abundances of p>12p>C and p>16p>O at the end of helium burning in stars.p>